The "Hubble" law of the velocity field for highly collimated bipolar outflows.

Details The "Hubble" law of the velocity field for highly collimated bipolar outflows. The "Hubble" law of the velocity field for highly collimated bipolar outflows.

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997acaps..17..291z&link_type=abstract

Acta Astrophys. Sin., Vol. 17, No. 3, p. 291 - 296

Astronomy and Astrophysics

Astrophysics

Star Formation: Molecular Outflows, Star-Forming Regions: Jets

Scientific paper

Among physical characteristics of highly collimated flows, the most important feature may be the "Hubble" law linking outflow velocity with distance from the driving source (v ∝ r). The bow shock driven by high-velocity jet may explain this relationship. A set of equations with variable ejecting angles is defined for the outflow shapes, velocity and density structure. The velocity field obtained by numerical method is comparable to the observations.

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